A model of holographic dark energy

被引：1625

作者：

Li, M

机构：

[1] Acad Sinica, Inst Theoret Phys, Beijing 100080, Peoples R China

[2] Acad Sinica, Interdisciplinary Ctr Theoret Studies, Beijing 100080, Peoples R China

来源：

PHYSICS LETTERS B | 2004年 / 603卷 / 1-2期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1016/j.physletb.2004.10.014

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A model for holographic dark energy is proposed, following the idea that the short distance cut-off is related to the infrared cut-off. We assume that the infrared cut-off relevant to the dark energy is the size of the event horizon. With the input Omega(Lambda) = 0.73, we predict the equation of state of the dark energy at the present time be characterized by w = -0.90. The cosmic coincidence problem can be resolved by inflation in our scenario, provided we assume the minimal number of e-foldings. (C) 2004 Elsevier B.V. All rights reserved.

引用

页码：1 / 5

页数：5

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